The WAGGS project-III. Discrepant mass-to-light ratios of Galactic globular clusters at high metallicity.

MLA

Dalgleish, H., et al. “The WAGGS Project-III. Discrepant Mass-to-Light Ratios of Galactic Globular Clusters at High Metallicity.” Monthly Notices of the Royal Astronomical Society, vol. 492, no. 3, Mar. 2020, pp. 3859–71. EBSCOhost, https://doi.org/10.1093/mnras/staa091.

APA

Dalgleish, H., Kamann, S., Usher, C., Baumgardt, H., Bastian, N., Veitch-Michaelis, J., Bellini, A., Martocchia, S., Da, C. G. S., Mackey, D., Bellstedt, S., Pastorello, N., & Cerulo, P. (2020). The WAGGS project-III. Discrepant mass-to-light ratios of Galactic globular clusters at high metallicity. Monthly Notices of the Royal Astronomical Society, 492(3), 3859–3871. https://doi.org/10.1093/mnras/staa091

Chicago

Dalgleish, H, S Kamann, C Usher, H Baumgardt, N Bastian, J Veitch-Michaelis, A Bellini, et al. 2020. “The WAGGS Project-III. Discrepant Mass-to-Light Ratios of Galactic Globular Clusters at High Metallicity.” Monthly Notices of the Royal Astronomical Society 492 (3): 3859–71. doi:10.1093/mnras/staa091.